First models of the s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver

@article{Lopez2021FirstMO,
  title={First models of the s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver},
  author={A. Yague L'opez and D. A. Garc'ia-Hern'andez and Paolo Ventura and C. L. Doherty and Jacqueline den Hartogh and S Jones and Maria Lugaro},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Aims. We describe the first s-process post-processing models for asymptotic giant branch (AGB) stars of masses 3, 4 and 5 M at solar metallicity (Z = 0.018) computed using the input from the stellar evolutionary code aton. Methods. The models are computed with the new code snuppat (S-process NUcleosynthesis Post-Processing code for aton), including an advective scheme for the convective overshoot that leads to the formation of the main neutron source, 13C. Each model is postprocessed with 3… 

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